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The Phillips spectrum and a model of wind-wave dissipation

机译:菲利普斯谱和风波耗散模型

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We consider an extension of the kinetic equation developed by Newell and Zakharov in 2008. The new equation takes not only the resonant four-wave interactions but also the dissipation associated with the wave breaking into account. In the equation, we introduce a dissipation function that depends on the spectral energy flux. This function is determined up to a functional parameter, which should be optimally chosen based on a comparison with experiment. A kinetic equation with this dissipation function describes the usually experimentally observed transition from the Kolmogorov-Zakharov spectrum E(omega) similar to omega(-4) to the Phillips spectrum E(omega) similar to omega(-5). The version of the dissipation function expressed in terms of the energy spectrum can be used in problems of numerically modeling and predicting sea waves.
机译:我们考虑了2008年开发的动力学方程的延伸。新的等式不仅需要谐振四波相互作用,而且占据了与播出的波浪相关的耗散。 在等式中,我们介绍了一种耗散函数,其取决于光谱能量通量。 该函数决定为功能参数,这应该基于与实验的比较来最佳选择。 具有这种耗散功能的动力学方程描述了与类似于ω(-5)的夏季谱E(ω)类似的Kolmogorov-Zakharov光谱E(Omega)的实验观察到的过渡。 以能谱表达的耗散函数的版本可用于数值建模和预测海波的问题。

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